Published by
EDP Sciences
EDP Sciences Journals List
Subscriber Authentication Point
Home All issues Volume 468/ 1 Article
Free access
Issue A&A
Volume 468, Number 1, June II 2007
Page(s) L25 - L28
Section Letters
DOI http://dx.doi.org/10.1051/0004-6361:20077294



A&A 468, L25-L28 (2007)
DOI: 10.1051/0004-6361:20077294

Letter

The water ice rich surface of (145453) 2005 RR $\mathsf{_{43}}$: a case for a carbon-depleted population of TNOs?

N. Pinilla-Alonso1, J. Licandro2, 3, R. Gil-Hutton4, and R. Brunetto5, 6

1  Fundación Galileo Galilei & Telescopio Nazionale Galileo, PO Box 565, 38700, S/C de La Palma, Tenerife, Spain
    e-mail: npinilla@tng.iac.es
2  Isaac Newton Group, 38700 Santa Cruz de La Palma, Tenerife, Spain
3  Instituto de Astrofísica de Canarias, c/Vía Láctea s/n, 38205 La Laguna, Tenerife, Spain
4  Complejo Astronómico El Leoncito (Casleo) and San Juan National University, Av. España 1512 sur, J5402DSP, San Juan, Argentina
5  Dipartimento di Fisica, Università del Salento, via Arnesano, 73100 Lecce, Italy
6  INAF-Osservatorio Astrofisico di Catania, via S. Sofia 78, 95123 Catania, Italy

(Received 13 February 2007 / Accepted 23 April 2007)

Abstract
Context.Recent results suggest that there is a group of trans-Neptunian objects (TNOs) (2003 EL61 being the biggest member), with surfaces composed of almost pure water ice and with very similar orbital elements. These objects provide exciting laboratories for the study of the processes that prevent the formation of an evolved mantle of organics on the surfaces of the bodies in the trans-Neptunian belt (TNb).
Aims.We study the surface composition of another TNO that moves in a similar orbit, (145453) 2005 RR43, and compare it with the surface composition of the other members of the group.
Methods.We report visible and near-infrared spectra in the 0.53-2.4 $\mu$m spectral range, obtained with the 4.2 m William Herschel Telescope and the 3.58 m Telescopio Nazionale Galileo at the "Roque de los Muchachos" Observatory (La Palma, Spain). Scattering models are used to derive information about its surface composition. We also measure the depth D of the water ice absorption bands and compare with those of the other members of the group.
Results.The spectrum of 2005 RR43 is neutral in color in the visible and dominated by very deep water ice absorption bands in the near infrared ( $D= 70.3 \pm 2.1$% and  $82.8 \pm 4.9\%$ at 1.5 $\mu$m and 2.0 $\mu$m respectively). It is very similar to the spectrum of the group of TNOs already mentioned. All of them present much deeper water ice absorption bands ($D >40 \%$) than any other TNO except Charon. Scattering models show that its surface is covered by water ice, a significant fraction in crystalline state with no trace (5% upper limit) of complex organics. Possible scenarios to explain the existence of this population of TNOs are discussed: a giant collision, an originally carbon depleted composition, or a common process of continuous resurfacing.
Conclusions.2005 RR43 is member of a group, may be a population, of TNOs clustered in the space of orbital parameters that show abundant water ice and no signs of complex organics and which origin needs to be further investigated. The lack of complex organics in their surfaces suggests a significant smaller fraction of carbonaceous volatiles like CH4 in this population than in "normal" TNOs. A carbon depleted population of TNOs could be the origin of the population of carbon depleted Jupiter family comets already noticed by A'Hearn et al. (1995).


Key words: Kuiper Belt -- solar system: formation



© ESO 2007

What is OpenURL?

The OpenURL standard is a protocol for transmission of metadata describing the resource that you wish to access. An OpenURL link contains article metadata and directs it to the OpenURL server of your choice. The OpenURL server can provide access to the resource and also offer complementary services (specific search engine, export of references...). The OpenURL link can be generated by different means.
  • If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
  • You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
  • You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.